A dataset provided by the European Space Agency

Name 085218
Title THE COMPTON THICK AGN LEGACY PROJECT: A COMPLETE SAMPLE OF NUSTAR-OBSERVED NEARB
URL

https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0852180101
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0852180201
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0852180301
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0852180401
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0852180501
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0852180601
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0852180701
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0852180801
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0852180901
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0852181001
https://nxsa.esac.esa.int/nxsa-sl/servlet/data-action-aio?obsno=0852181201
...

DOI https://doi.org/10.5270/esa-xkxmqtu
Author European Space Agency
Description The X-ray spectral analysis of Compton thick (CT, having intrinsic obscuration
NH>1E24 cm^-2) active galactic nuclei (AGN) is key to understand the physics of
the obscuring material surrounding accreting supermassive black holes. We pro-
pose to target with a combined NuSTAR/XMM-Newton observation the last 10 can-
didate CT-AGN the BAT 100-month survey still lacking of NuSTAR data. With this
proposal, each CT-AGN candidate of this sample will have a NuSTAR observation,
thus enabling the best characterization to date of CT-AGN. Thanks to the ex-
cellent statistics (both in terms of spectral counts and sample size) we will
study the sample physical properties, and put tighter constraints on the true
intrinsic fraction of CT-AGN in the nearby Universe and on contribution to CXB.
Publication No observations found associated with the current proposal
Instrument EMOS1, EMOS2, EPN, OM, RGS1, RGS2
Temporal Coverage 2019-08-20T17:26:30Z/2020-02-24T00:21:34Z
Version 18.02_20200221_1200
Mission Description The European Space Agency's (ESA) X-ray Multi-Mirror Mission (XMM-Newton) was launched by an Ariane 504 on December 10th 1999. XMM-Newton is ESA's second cornerstone of the Horizon 2000 Science Programme. It carries 3 high throughput X-ray telescopes with an unprecedented effective area, and an optical monitor, the first flown on a X-ray observatory. The large collecting area and ability to make long uninterrupted exposures provide highly sensitive observations.
Since Earth's atmosphere blocks out all X-rays, only a telescope in space can detect and study celestial X-ray sources. The XMM-Newton mission is helping scientists to solve a number of cosmic mysteries, ranging from the enigmatic black holes to the origins of the Universe itself. Observing time on XMM-Newton is being made available to the scientific community, applying for observational periods on a competitive basis.
Creator Contact https://www.cosmos.esa.int/web/xmm-newton/xmm-newton-helpdesk
Date Published 2021-03-17T00:00:00Z
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, 2021, The Compton Thick Agn Legacy Project: A Complete Sample Of Nustar-Observed Nearb, 18.02_20200221_1200, European Space Agency, https://doi.org/10.5270/esa-xkxmqtu